Quantum Quench and Thermalization in Free Scalar Field Theory and its Gravity Dual (In Arbitrary Dimensions)

dc.contributor.advisorMandal, Gautamen_US
dc.contributor.authorBANERJEE, PARIJATen_US
dc.contributor.departmentDept. of Physicsen_US
dc.contributor.registration20131010en_US
dc.date.accessioned2018-05-24T10:37:50Z
dc.date.available2018-05-24T10:37:50Z
dc.date.issued2018-05en_US
dc.description.abstractIn this work we explore the thermalization of two point functions of free scalars in $d+1$ dimensions after a quantum quench. The mass is time dependent and is taken to zero. A detailed analysis of this problem has been done in 1+1 dimensions, in \cite{Mandal:2015kxi}. My goal here is to extend this understanding to higher dimensions. In previous works,\cite{Mandal:2015jla}\cite{Mandal:2015kxi}, we have seen that the post quench system equilibriates to a generalised Gibb's Ensemble. The post-quench observables retain a memory of the quench by having signatures set by the scale of the pre-quench state. We restrict our calculations to two kinds of pre-quench states: the ground state of the pre-quench Hamiltonian, and specific excited states called the squeezed states (CC and GCC). \par All observables seem to reach an equilibrium. The correlation functions in the CC approach a thermal ensemble and those in the GCC approach a GGE, at late times, and are related by, $\beta=4\kappa_2$ and $\mu=4\kappa_4$. We observe a distinction between odd and even dimensions. The approach to equilibrium is exponentially decaying in time for odd $d$ and fall off as a power law for even $d$. We also calculate the time dependent thermal correlator and observe a similar difference in odd and even dimensions. \par In the second last section, we discuss the possibility of UV-IR mixing in the GCC and GGE. The post-quench state is characterized by infinite number of conserved charges which may correspond to irrelevant operators in the theory. Observables seem to be affected by all such operators even at low energies, which is interesting given our intuitions set by Wilsonian renormalization. \par Finally, we wish to understand the implications of this result in the context of holography, with the knowledge that thermalization in the gauge theory corresponds to a quasi-normal decay to a black-hole. A quench itself can correspond to an excitation in the bulk.en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/1046
dc.language.isoenen_US
dc.subject2018en_US
dc.subjectPhysicsen_US
dc.subjectQuantum Quenchen_US
dc.subjectHolographyen_US
dc.subjectTwo point functionsen_US
dc.subjectThermalizationen_US
dc.subjectCalabrese-Cardyen_US
dc.subjectGeneralised Gibb's Ensembleen_US
dc.titleQuantum Quench and Thermalization in Free Scalar Field Theory and its Gravity Dual (In Arbitrary Dimensions)en_US
dc.typeThesisen_US
dc.type.degreeBS-MSen_US

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